Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes
Autor(a) principal: | |
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Data de Publicação: | 2021 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
Texto Completo: | http://hdl.handle.net/10071/22675 |
Resumo: | We compute the quasinormal frequencies of d-dimensional spherically symmetric black holes with leading string corrections in the eikonal limit for tensorial gravitational perturbations and scalar test fields. We find that, differently than in Einstein gravity, the real parts of the frequency are no longer equal for these two cases. The corresponding imaginary parts remain equal to the principal Lyapunov exponent corresponding to circular null geodesics, to first order in . We also compute the radius of the shadow cast by these black holes. |
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Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holesWe compute the quasinormal frequencies of d-dimensional spherically symmetric black holes with leading string corrections in the eikonal limit for tensorial gravitational perturbations and scalar test fields. We find that, differently than in Einstein gravity, the real parts of the frequency are no longer equal for these two cases. The corresponding imaginary parts remain equal to the principal Lyapunov exponent corresponding to circular null geodesics, to first order in . We also compute the radius of the shadow cast by these black holes.Elsevier2021-06-07T13:33:04Z2021-01-01T00:00:00Z20212021-06-07T14:31:44Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10071/22675eng0370-269310.1016/j.physletb.2021.136407Moura, F.Rodrigues, J.info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-11-09T18:00:08Zoai:repositorio.iscte-iul.pt:10071/22675Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T22:31:48.460174Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse |
dc.title.none.fl_str_mv |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
title |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
spellingShingle |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes Moura, F. |
title_short |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
title_full |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
title_fullStr |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
title_full_unstemmed |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
title_sort |
Eikonal quasinormal modes and shadow of string-corrected d-dimensional black holes |
author |
Moura, F. |
author_facet |
Moura, F. Rodrigues, J. |
author_role |
author |
author2 |
Rodrigues, J. |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Moura, F. Rodrigues, J. |
description |
We compute the quasinormal frequencies of d-dimensional spherically symmetric black holes with leading string corrections in the eikonal limit for tensorial gravitational perturbations and scalar test fields. We find that, differently than in Einstein gravity, the real parts of the frequency are no longer equal for these two cases. The corresponding imaginary parts remain equal to the principal Lyapunov exponent corresponding to circular null geodesics, to first order in . We also compute the radius of the shadow cast by these black holes. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-06-07T13:33:04Z 2021-01-01T00:00:00Z 2021 2021-06-07T14:31:44Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10071/22675 |
url |
http://hdl.handle.net/10071/22675 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
0370-2693 10.1016/j.physletb.2021.136407 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier |
publisher.none.fl_str_mv |
Elsevier |
dc.source.none.fl_str_mv |
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Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
collection |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
repository.name.fl_str_mv |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
repository.mail.fl_str_mv |
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1799134879548440576 |